Show simple item record

Files in this item

Thumbnail

Item metadata

dc.contributor.authorErcolano, Barbara
dc.contributor.authorKoepferl, Christine
dc.contributor.authorOwen, James
dc.contributor.authorRobitaille, Thomas
dc.date.accessioned2016-02-19T16:40:09Z
dc.date.available2016-02-19T16:40:09Z
dc.date.issued2015-10-01
dc.identifier.citationErcolano , B , Koepferl , C , Owen , J & Robitaille , T 2015 , ' Far-infrared signatures and inner hole sizes of protoplanetary discs undergoing inside-out dust dispersal ' , Monthly Notices of the Royal Astronomical Society , vol. 452 , no. 4 , pp. 3689-3695 . https://doi.org/10.1093/mnras/stv1528en
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 241104230
dc.identifier.otherPURE UUID: 7d122ded-4cbf-4a7c-b90d-809fbcac3673
dc.identifier.otherBibCode: 2015MNRAS.452.3689E
dc.identifier.otherScopus: 84940121792
dc.identifier.urihttp://hdl.handle.net/10023/8269
dc.descriptionJEO acknowledges support by NASA through Hubble Fellowship grant HST-HF2-51346.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555.en
dc.description.abstractBy means of radiative transfer simulation, we study the evolution of the far-infrared colours of protoplanetary discs undergoing inside-out dispersal, often referred to as transition discs. We show that a brightening of the mid- and far-infrared emission from these objects is a natural consequence of the removal of the inner disc. Our results can fully explain recent observations of transition discs in the Chamaleon and Lupus star-forming regions from the Herschel Gould Belt Survey,which shows a higher median for the 70 μm (Herschel PACS 1) band of known transition objects compared with primordial discs. Our theoretical results hence support the suggestion that the 70 μm band may be a powerful diagnostic for the identification of transition discs from photometry data, provided that the inner hole is larger than tens of au, depending on spectral type. Furthermore, we show that a comparison of photometry in the K, 12 μm and 70 μm bands to model tracks can provide a rough, but quick estimate of the inner hole size of these objects, provided their inclination is below ˜85° and the inner hole size is again larger than tens of au.
dc.format.extent7
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Societyen
dc.rights© 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at https://dx.doi.org/10.1093/mnras/stv1528en
dc.subjectProtoplanetary discsen
dc.subjectQB Astronomyen
dc.subjectQC Physicsen
dc.subjectNDASen
dc.subject.lccQBen
dc.subject.lccQCen
dc.titleFar-infrared signatures and inner hole sizes of protoplanetary discs undergoing inside-out dust dispersalen
dc.typeJournal articleen
dc.description.versionPublisher PDFen
dc.contributor.institutionUniversity of St Andrews.School of Physics and Astronomyen
dc.identifier.doihttps://doi.org/10.1093/mnras/stv1528
dc.description.statusPeer revieweden
dc.identifier.urlhttp://adsabs.harvard.edu/abs/2015MNRAS.452.3689Een


This item appears in the following Collection(s)

Show simple item record